Coupled dark energy with perturbed Hubble expansion rate
Yang, WQ ; Xu, LX
刊名PHYSICAL REVIEW D
2014
卷号90期号:8页码:83532
关键词OSCILLATION SPECTROSCOPIC SURVEY BARYON ACOUSTIC-OSCILLATIONS INTERACTING QUINTESSENCE REDSHIFT-SPACE GROWTH-RATE MODELS MATTER CONSTRAINTS GALAXIES PERTURBATIONS
ISSN号1550-7998
通讯作者Yang, WQ (reprint author), Dalian Univ Technol, Sch Phys & Optoelect Technol, Inst Theoret Phys, Dalian 116024, Peoples R China.
英文摘要The coupling between dark sectors provides a possible approach to mitigate the coincidence problem of the cosmological standard model. In this paper, dark energy is treated as a fluid with a constant equation of state, whose coupling with dark matter is proportional the Hubble parameter and energy density of dark energy, that is, (Q) over bar = 3 xi(x)(H) over bar(rho) over bar (x). In particular, we consider the Hubble expansion rate to be perturbed in the perturbation evolutions of dark sectors. Using joint data sets which include cosmic microwave background radiation, baryon acoustic oscillation, type Ia supernovae, and redshift-space distortions, we perform a full Markov chain Monte Carlo likelihood analysis for the coupled model. The results show that the mean value with errors of the interaction rate is xi(x) = 0.00305(-0.00305-0.00305-0.00305)(+0.000645+0.00511+0.00854) for Q(A)(mu)parallel to u(c)(mu) and xi(x) = 0.00317(-0.00317-0.00317-0.00317)(+0.000628+0.00547+0.00929) for Q(A)(mu)parallel to u(x)(mu), which means that the recent cosmic observations favor a small interaction rate which is up to the order of 10(-3). Moreover, in contrast to the coupled model with an unperturbed expansion rate, we find the perturbed Hubble expansion rate can bring about a negligible impact on the model parameter space.
学科主题Physics
收录类别SCI
资助信息NSFC [11275035]; Fundamental Research Funds for the Central Universities [DUT13LK01]
原文出处http://dx.doi.org/10.1103/PhysRevD.90.083532
语种英语
WOS记录号WOS:000350215700001
公开日期2015-06-03
内容类型期刊论文
源URL[http://ir.itp.ac.cn/handle/311006/15599]  
专题理论物理研究所_理论物理所1978-2010年知识产出
推荐引用方式
GB/T 7714
Yang, WQ,Xu, LX. Coupled dark energy with perturbed Hubble expansion rate[J]. PHYSICAL REVIEW D,2014,90(8):83532.
APA Yang, WQ,&Xu, LX.(2014).Coupled dark energy with perturbed Hubble expansion rate.PHYSICAL REVIEW D,90(8),83532.
MLA Yang, WQ,et al."Coupled dark energy with perturbed Hubble expansion rate".PHYSICAL REVIEW D 90.8(2014):83532.
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